List of Figures Figure 5 The fully developed velocity profile compares with the Navior-Stokes solution in Poiseuille flow……….……...28 simple DPD fluid in Poiseuille flow……….……….…...29 Fig
Trang 1DISSIPATIVE PARTICLE DYNAMICS SIMULATION OF MICRO-CONCENTRIC/ECCENTRIC ANNULAR FLOWS
PENGFEI CHEN
A THESIS SUBMITTED FOR THE DEGREE OF MASTER OF ENGINEERING
DEPARTMENT OF MECHANICAL ENGINEERING
NATIONAL UNIVERSITY OF SINGAPORE
2004
Trang 2ACKNOWLEDGEMENTS
I am very grateful to my supervisors, Professor Nhan Phan-Thien and Associate
Professor Yeo Khoon Seng for giving me the great opportunity to study in such an
interesting area I would also like to express my sincere gratitude to them for their
constant guidance and encouragement throughout the course of this work
I would like to thank Professor Fan Xijun, Dr Dou Huashu, Dr Chen Shuo, Dr Lu
Zhumin, Dr Shi Xing, Mr Wu Tao, Ms Luo Chunshan and Ms Zhao Xijing for their
assistance and friendship
My entire family deserves a special gratitude for their unlimited support,
encouragement and love throughout my stay in NUS
Finally, I would like to give my acknowledgement to the National University of
Singapore for their Research Scholarship
Thanks are also due to all others who have helped me in one way or another in this
effort
Trang 3Table of Contents
Acknowledgement I
Summary IV
Nomenclature V
List of Figures VIII
List of Tables XII
Chapter 1 Introduction 1
1.1 Background …… 1
1.2 Literature review …… 4
1.3 Objective of this research project …… 6
Chapter 2 Methodology 9
2.1 Basic equations of DPD method …… 9
2.2 Numerical Scheme …… 14
2.3 Initial Particle Models in concentric/eccentric flow field 16
Chapter 3 Steady Concentric/eccentric flows of simple DPD fluids at finite Reynolds numbers …… 20
3.1 Implementation of non-slip boundary condition in DPD 21
3.1.1 Boundary condition used in this thesis……… 24
3.1.2 Comparison of boundary conditions: Poisseuille flow… 26
3.1.3 Comparison of boundary conditions: Concentric rotating
Trang 43.2 Effects of some DPD Parameters on simulation……… 32
3.2.1 Effect of fluid particle density……….………33
3.2.2 Effect of conservative force factor between DPD particles……….……… 36
3.3 Steady Circular Couette flow and eccentric flow of simple DPD fluids at finite Reynolds numbers……… ……… 43
3.3.1 Circular Couette flow of simple DPD fluids at finite Reynolds numbers……….… 43
3.3.2 Eccentric flow (ωout/ωin=0) of simple DPD fluids at finite Reynolds numbers……….… 48
Chapter 4 Steady Circular/eccentric flows of FENE Chain Suspension at finite Reynolds numbers……….…………60
4.1 Circular Couette flow of FENE chain suspension at finite Reynolds numbers……… 62
4.2 Eccentric flow (ωout/ωin=0) of FENE chain suspension at finite Reynolds numbers……… ……… 70
Chapter 5 Conclusion and future works …… ….80
5.1 Conclusion………… ……… …80
5.2 Future works……….……….81
Appendix A……….……… … 84
Appendix B……… … 87
Reference………88-92
Trang 5Summary
Dissipative Particle Dynamics (DPD) is a fairly new method for simulating complex
fluid flows and other colloidal phenomena It is a mesoscopic method and offers the
possibility of capturing some degree of molecular-level detail while conforming to
continuum hydrodynamics at larger length scales In this thesis, a new implementation
of the no slip boundary condition in the modeling of solid boundaries is studied This
boundary is implemented to simulate the planar Poisseuille and circular Couette flow,
and the results compare excellently with similar results derived by more traditional
CFD methods The effects of two important DPD parameters (particle density and
conservative coefficient) are studied It is shown that these two parameters affect the
simulation accuracy considerably and should be carefully set Furthermore, to confirm
the ability of DPD method to provide numerically accurate results in simulating
complex flow with rather complicated boundary conditions, the DPD method is
employed to study the flow behavior of three dimensional microscopic
concentric/eccentric flows at finite Reynolds numbers A simple DPD fluid (made up
of simple DPD particles) and then bio-molecular suspensions (FENE chains are used to
model DNA macromolecules) are studied in detail respectively
Trang 6Nomenclature
It is not practical to list all the symbols that have been used Below the author list the
more important ones Some of the symbols are defined as they are used There are also
occasions where the same symbol is assigned a different meaning in a different context,
but the meaning should normally be clear from the usage
Trang 7Rin Radius of inner cylinder
Trang 8ρ Fluid density
c Mean annular gap width, Rout-Rin
Trang 9List of Figures
Figure 5 The fully developed velocity profile compares with the Navior-Stokes
solution in Poiseuille flow……….…… 28
simple DPD fluid in Poiseuille flow……….……….… 29
Figure 10 The comparison of pressure profiles in Poiseuille flow……… 30
Figure 11 The comparison of velocity profiles of a simple DPD fluid in circular
Couette flow……….…32
Figure 12 Illustration of the effect of fluid particle density on velocity of a simple
DPD fluid in circular Couette flow……….….34
Figure 13 Comparison of temperature profiles of a simple DPD fluid in circular
Figure 14 Comparison of density profiles of a simple DPD fluid in circular Couette
Trang 10Figure 15 Comparison of velocity profiles of a simple DPD fluid in circular Couette
circular Couette flow……….……….… 41
Figure 17 Comparison of temperature profiles of a simple DPD fluid in circular
Figure 18 Comparison of velocity profiles of a simple DPD fluid in circular Couette
Figure 19 Geometry for Circular Couette flow……….… 43
Figure 20 Simulated Vx, Vz velocity and streamline contours of a simple DPD fluid
in circular Couette flow……… 45
Figure 21 The fully developed tangential velocity profile of a simple DPD fluid in
circular Couette flow……….……… 46
Figure 22 Density and temperature profiles of a simple DPD fluid in circular Couette
flow……… …46
Figure 23 Pressure profile of a simple DPD fluid in circular Couette flow…….…47
Figure 24 Shear stress distribution of a simple DPD fluid in circular Couette
flow……… 47
Figure 25 Profiles of the first and second normal stress differences of a simple DPD
fluid in circular Couette flow……… ….48
Figure 26 Bipolar coordinate system and geometric parameters of the eccentric
annular region……… 50
Trang 11Figure 27 Streamline patterns of a simple DPD fluid in eccentric flow (ωout/ωin=0)
with different Reynolds numbers……….………….58
Figure 28 Comparison of polar angles of separation and reattachment points of
Figure 31 Comparison of velocity profiles of FENE chain suspensions of different
concentrations in the Circular Couette flow……….…….64
Figure 32 Comparison of pressure profiles of FENE chain suspensions of different
concentrations in the Circular Couette flow……….……….65
Figure 33 Comparison of Shear stress profiles of FENE chain suspensions of
different concentrations in the Circular Couette flow……….…… 65
Figure 34 The conformation of some typical FENE chains in circular Couette flow
Trang 12(ωout/ωin=0) with different volume fractions……….………….73
Figure 39 Illustration plot of the development of the back flow of FENE chain
Figure 40 Snapshots showing the detailed backflow of one FENE chain in eccentric
flow……… 79
Trang 13List of Tables
fractions……… 73
Trang 14Chapter 1 Introduction 1.1 Background
The numerical simulation of hydrodynamic interactions between suspended particles
and the surrounding fluid phase is of interest in many engineering applications
associated with particle transport, such as colloids, polymers, aerosols and
physiological system [1] The properties of these systems are often determined by
their mesoscale structures, i.e between the atomistic scale and the macroscopic scale,
thus endowing a complex fluid with unique and interesting features [2]
Dynamic simulation of these systems presents unique problems that are difficult to
address with established methods On the one hand, the time and length scales of
interest make simulation by molecular dynamics (MD) impractical, a limitation that is
not likely to be solved in the near future, even with the rapid increases in
computational speed that are expected to develop On the other hand, colloidal length
scales are often almost the same order as the flow domain size (The ratio of the
colloidal length to the characteristic length of flow field can be taken as the equivalent
continuum) So purely continuum approaches, such as conventional computational
fluid dynamics (CFD), are unacceptable, requiring as they do that one leaves out so
many details at the molecular level Moreover, people still cannot make the full
connection from atomistic length-scale to the macroscopic world Hence to obtain a
better understanding of the phenomena that occur in mesocale, some intermediate
Trang 15simulation techniques are developed that are aimed at a length-scale larger than the
atomistic scale, but smaller than the macroscopic scale Dissipative particle dynamics
(DPD) is a so-called mesoscopic simulation method that provides one possible means
of bridging the gap between purely molecular and continuum-level treatments
Dissipative particle dynamics is a stochastic simulation technique introduced by
Hoogerbrugge and Koelman [3] in 1992 to simulate complex fluid dynamical
phenomena DPD combines features from molecular dynamics and lattice-gas
automata (LGA) by introducing a LGA-type of time-stepping into MD schemes In
contrast to molecular dynamics simulations, the particles are supposed to represent the
fluid on a mesoscopic level rather than a molecular level For the simulation of
macroscopic fluid dynamic phenomena, this implies an advantage of computational
effort [4] Though Brownian Dynamics Simulation (BDS), LGA and Lattice
Boltzmann (LB) are mesoscale simulation methods, it is difficult for BDS to deal with
complex flow field and for LGA and LB to cope with complex fluids and DPD has the
advantage of more flexibility
The basic unit in DPD system is a set of discrete momentum carriers called particles
that move in continuous space and discrete time-steps The momentum carriers are
coarse grained entities which are no longer regarded as molecules in a fluid but rather
representing the collective dynamic behavior of a large number of molecules (a fluid
Trang 16Particle Dynamics is such a method for simulation of the motion of this kind of “fluid
particles” often referred to in continuum mechanics Conceptually this method
amounts to dividing up the molecules of a flow field into groups or packets, which
have dimensions many times larger than the mean free path of an individual molecule
The mass m of each packet is localized to a point As the points move, their interaction
is ‘soft’ as a result of the fact that the packets are deformable, and this deformation is
accompanied by a dissipation of energy In addition, because of their small
colloid-like dimensions, the thermal motion of the molecules in the packets gives rise
to a random or Brownian contribution to their motion A time step in a DPD
simulation therefore consists of summing interactions that consist of three terms: a
conservative repulsion that accounts for steric and energetic interactions between the
molecules of interacting packets and this repulsion force prevents particles from
overlapping [5], a dissipative interaction that accounts for energy that is lost due to
internal friction or viscosity within a packet, and a random step that arises from the
collective thermal motion of the molecules within a packet The interactions are
summed over all pairs of particles, in a way that guarantees that linear and angular
momentum are conserved Unless an explicit connection to molecular-level
interactions is needed, the parameters that govern these interactions are chosen in any
way that reproduces the continuum-level dimensionless groups that determine the
behavior of a particular system
The last two terms, which account for dissipation and random motion, are necessarily
Trang 17coupled by a fluctuation-dissipation theorem and the principle of equipartition of
energy These two terms combine to create a continuous pseudofluid in which the
particles are suspended and free to interact hydrodynamically The original algorithm
of Hoogerbrugge and Koelman [3] did not satisfy this requirement, leaving in doubt
whether a simulation could reach a true equilibrium, even at long times and in the
absence of bulk motion A slight revision of the original algorithm, produced by
Espanol and Warren [6], remedied this problem, and has been used in most
applications since that time The method has received considerable theoretical support
in other areas as well Marsh et al [7] make explicit connections between DPD and
the Navier-Stokes equations by deriving the Fokker-Planck-Boltzmann equation for
the single-particle distribution function, and solving it by the Chapman-Enskog
method Their derivation includes expressions for transport properties such as the
shear viscosity that are valid in the limit of strong damping, where conservative
repulsive interactions are negligible Flekkoy and Coveney [8] discussed creating
DPD particles by grouping molecules in MD simulations together
1.2 literature review
Since DPD method is a fairly recent development and the method is still evolving,
only the fundamental and representative papers will be reviewed here Literature
review about the flow field in concentric/eccentric flows will be noted in the section
on results and discussion
Trang 18A key and attractive feature of DPD is its ability to reproduce continuum-level fluid
mechanics over large enough length scales, even in the presence of inertia However,
in spite of the growing literature on the applications of DPD to various problems,
there are still relatively few direct, quantitative comparisons between calculations
done with DPD and well-established analytical and numerical results Those
comparisons that do exist pertain exclusively to low Reynolds numbers
Simulation results obtained by DPD have also been reported for several problems of
interests In their original paper, Hoogerbrugge and Koelman [3] calculated the
flow-induced drag on a cylinder in a periodic array, and compared it with result
reported by Sangani and Acrivos [9] This comparison was made in the limit of low
Reynolds number, where inertial effects in the flow are negligible Boek et al [10, 11]
studied the rheological properties of colloidal suspensions of spheres and rods using
dissipative particle dynamics, and measured the viscosity as a function of shear rate
and volume fraction of the suspended particles Furthermore Boek and van der Schoot
[12] used DPD to study fluid flow through a periodic array of cylinders as a model for
fluid filtration through a porous medium, and discussed the resolution effects in DPD
Both the calculations of Hoogerbrugge and Koelman [3] and those of Boek et al [10,
11, 12] were done with the original algorithm, without the modification proposed by
Espanol and Warren [6]; Boek et al [12] argued that the modification does not
significantly alter the calculations of suspension rheology Model polymers have been
Trang 19constructed by linking DPD particles together with springs, and polymer dynamics
and associated parameters have been studied by Kong et al [13] In addition,
polymer-surfactant aggregation and micelle formation have been simulated by Groot
[14], and an extension of DPD to non-Newtonian flows (Bosch [4]) has been proposed
More recently, Fan et al [15] presented their simulation results for macromolecular
suspension flows through microchannels They also studied the Poiseuille flow of
simple DPD fluids and FENE (Finitely Extendable Nonlinear Elastic) chains
suspension and found that simple DPD fluids behave just like a Newtonian fluid while
FENE chains suspension can be fitted by dilute suspensions
1.3 Objective of this research project
As noted above, DPD has its own advantages to numerically simulate the
hydrodynamic interactions of various complex systems: such as polymer suspensions
[13, 16, 17, 18], colloids [10, 11, 19] and multiphase fluids [20, 21, 22] Although it is
a promising technique for complex fluids, there are very few microfluidic applications
of DPD in complex systems reported The most recent literature that combines such a
microscopic application of DPD in complex system as well as giving a quantitative
simulation is noted in the paper of Fan et al [15], but what is studied in their paper is
about the simple Poiseuille flow In this thesis, a more complex flow problem is
studied: steady microscopic concentric/eccentric flow at finite Reynolds numbers
This work is also stimulated by the recent innovations in MEMS devices, especially in
Trang 20understood today
Unlike the Poiseuille flow, firstly, the boundary condition of concentric/eccentric flow
is more complicated because it is a closed flow field and the implementation of the
boundary conditions will have a more significant impact on the simulation results
Secondly, the flow patterns in concentric/eccentric flows are more intricate compared
with that of Poiseuille flow at low Reynolds numbers, especially for eccentric flow
(there is a clear recirculation region present in the flow field) Same with what are
presented in the paper of Fan et al., two kinds of fluids are studied here: simple DPD
fluids and FENE chains suspension Some results on the deformation and migration of
FENE are also reported
It should be noted that the purpose of this research program is not to propose DPD as
an instrument for use in computational fluid mechanics, but rather to test its ability to
capture continuum fluid mechanical effects in the presence of significant inertia Even
capture inertial effects accurately is important In their study of the Brownian motion
corrections to the equations of motion for each frequency of oscillation They found a
nonlinear force of interaction between the particles that, even for very small Reynolds
and temperature, and R is the particle radius Such an interaction has an effect on the
distribution of the particles, which in turn affects the thermodynamics and rheological
Trang 21properties of a colloidal suspension
Since fluid simulation by DPD is a fairly new development, the results presented in
this thesis are focused on a number of test problems These problems include:
improving the dynamic behavior of DPD method, studying the effects of basic DPD
parameters (α and n) on simulation results, and accessing the ability of DPD to
provide numerically accurate results in simulating complicated flows with
complicated boundary conditions The simulation results presented in this work
confirm the ability of DPD to provide quantitatively accurate results for complicated
flows, provided conditions are such that the compression of the DPD fluid is not
significant
In the present work, the DPD method is used to calculate three-dimensional flows at
finite Reynolds numbers, and examine conditions under which Newtonian fluid and
non-Newtonian fluid behaviour is reproduced quantitatively First, the DPD method is
outlined This is followed by the description of a new implementation of DPD
boundary condition, and then the effects of DPD parameters are studied, with some
simulation details presented The simulation details for concentric/eccentric flows
with simple DPD fluids and FENE chains suspensions are presented next
Trang 22Chapter 2 Methodology 2.1 Basic equations of DPD method
The DPD system consists of a set of interacting “particles”, whose time evolution is
mass is taken to be the mass of a particle, so that the force acting on a particle is
particle i by particle j , which is assumed to be pairwise additive The dynamic
interactions between the particles are composed of two parts, dissipative and
stochastic, complementing each other to ensure a constant value for the mean kinetic
ij ij j
i ij
ij F F F
≠
(2)
Since the time average of the dissipative and fluctuation forces is zero, they do not
feature in the equilibrium behavior of the system, which is governed solely by
Trang 23along the line of centers and is given by
C
ˆ(1 / ) ( )
ij
ˆ( )(ˆ )
ij = −γw r ij ij⋅ ij ij
ij= −i j
characterizing the extent of dissipation in a single simulation step The negative sign
step:
( ) 0
ij t
Trang 24over a time scale considerably larger than its correlation time scale:
The detailed balance condition, similar to a Fluctation-Dissipation theorem relating
the strength of the random force to the mobility of a Brownian particle, requires that
will ensure that the temperature remains constant
We use the following weight function to improve on the Schmidt number for the
This weight function yields a stronger dissipative force between particles than that
from the standard quadratic force for a given configuration of particles and
interaction strength
ij
F ,
hand, reduces the relative velocity of two particles and removes kinetic energy from
their mass centre to cool the system down When the detailed balance is reached, the
Trang 25system temperature will approach the given value The dissipative and random
forces act like the thermostat in molecular dynamics (MD)
When simulating complex fluids and flows, simple DPD particles, described above,
are used to model solvent or suspending fluid The solid walls can be modeled by
frozen DPD particles The Finitely Extendable Nonlinear Elastic (FENE) chain is a
model commonly used to model flexible polymer molecules in rheology; it is used in
this thesis to model bio-molecules Beads of the polymer chain are replaced by DPD
particles The intermolecular forces will act on these particles and should be added to
the right hand side of Eq (1)
In the FENE chain [24], the force on bead i due to bead is j is
2
ij S
/
ij m
predict a shear-rate dependent viscosity and finite elongational viscosity The mass
of the beads is assumed to be unity, which is as same as that of other simple DPD
fluid particles
Trang 26The time constant is important in characterizing molecular motion and can be
formed from model parameter Two constants with the time dimension can be
obtained for the FENE spring [24],
k T
λλ
Chain models usually have a spectrum of relaxation times [24] There is no closed
form expression for the relaxation time spectrum for FENE chains; however, a
modification of FENE chain, called the FENE-PM chain, has the same spectrum as
the Rouse chain (bead and Hookean spring chain) [24] A time constant can be
defined for FENE-PM chain as [25]:
2
1
b fene H
N b
b
The contour length is an appropriate parameter to represent the molecular size If
c
Trang 27m c
r L
b
=
2.2 Numerical Scheme
The initial configuration of fluid and wall particles are generated separately by a
pre-processing program and read in as input data The total number of particles
depends on the size and geometry of the flow domain, the densities of the fluid and
wall materials The initial velocities of fluid particles are set randomly according to
the given temperature but the wall particles are frozen At the beginning of the
simulation the particles are allowed to move without applying the external force and
rotation until the thermodynamic equilibrium state is reached Then the rotating
velocity is applied to the inner or outer cylinder wall particles and the
non-equilibrium simulation starts
The forces computation and time updates are conducted with Cartesian coordinate
system and the samples averaging work are carried out with polar coordinate system
for concentric flow and double-polar coordinate system for eccentric flow
Since the dissipative force is dependent on the velocity, a modified version of the
velocity-Verlet algorithm [26] is used This algorithm can be described as follows:
Trang 28which account for some additional effects of the stochastic interactions If the total
force is velocity independent, the standard velocity-Verlet algorithm is recovered for
λ =0.5 Groot and Warren [26] found that the optimum value of λ is 0.65 For this
Trang 29equation describes the contribution to the stress from the momentum transfer of DPD
particles and the second term from the interparticle forces For simple DPD particle
13
p= − trS (21)
2.3 Initial Particle Models in concentric/eccentric flow field
Since we assume that the purpose of the simulation is to study the equilibrium fluid
state, then the nature of the initial particle configuration should have no influence
whatsoever on the outcome of the simulation In choosing the initial coordinates, the
usual method is to position the atoms at the sites of a lattice whose unit cell size is
chosen to ensure uniform coverage of the simulation region Typical lattices used in
three dimensions are the face-centered cubic(FCC) and simple cubic, whereas in two
dimensions the square and triangular lattices are used; if the goal is the study of the
solid state, then this will dictate the lattice selection There is little point in
laboriously constructing a random arrangement of atoms, typically using a Monte
Carlo procedure to avoid overlap, since the dynamics will produce the necessary
randomization very quickly An obvious way of reducing equilibration time is to
base the initial state on the final state of a previous run
Trang 30The function of FCC arrangement (with the optional of unequal edges) is to generate
four particles per unit cell To generate more particles in one cell, there are other
arrangement methods For example, the diamond lattice, which can generate eight
particles per unit cell, is a slightly more complicated form of the FCC code since the
lattice is most readily defined as two staggered FCC lattices, one of which is offset
along the diagonal by a quarter unit cell Similarly, to distribute 12 particles in one
unit cell, three staggered FCC lattices can be built up with offset of 0.125 unit cell
These three arrangements are used in this thesis to generate the required particle
(1) Fluid Particle disposition
First, particles are distributed evenly in a prism whose square section is bigger than
the outer circle; then deduct particles outside of the outer circle and particles within
the inner circle, and the shade area shown in Figure 1 represents the needed flow
domain
In this three-dimensional problem, the periodic boundary condition is applied to
fluid boundaries of the axis direction, which is y direction of Figure 1 Particles that
leave the simulation region of y direction immediately reenter the region through the
opposite face For this steady, low Reynolds number case, this application of
periodic boundary condition is workable and feasible
Trang 31Figure 1 Illustration of generating fluid particles in an annular area
(2) Wall Particle disposition
Solid walls are modeled by frozen DPD particles; three wall layers with staggered
distribution in angular (Fig.2) and radial (Fig 3) directions
Due to the soft interaction between DPD particles, it is difficult to prevent particles
from penetrating the wall if the wall particle density is too low compared with the
fluid particle density; however, a higher density of the wall will produce a stronger
repulsive force between the wall DPD particles and fluid DPD particles, and
consequently a large density fluctuation appears near the wall So normally the wall
particle density is chosen to be of the same order of that of fluid particles
X
Y
Z
Trang 32On the other hand, the repulsive force between wall particles and fluid particles is
also determined by the value of repulsive force coefficient between them So the
wall particle density should be set rationally, although there is no certain mode to
distribute the wall particles for such a special wall boundary contour
Figure 2 Illustration of generating wall
particles in angular direction
Figure 3 Illustration of generating wall particles in radial direction
Trang 33Chapter 3 Steady Concentric/eccentric flows of simple
DPD fluids at finite Reynolds numbers
Some of implementation details on DPD are briefly introduced here The program is
usually divided into 2 parts: a pre-processing program and a main one In
pre-processing program, the initial particle configurations for the fluid, wall and
DNA chains (if any) are generated and read into the main program as input data
When the density of fluid and the geometry of flow domain are defined, the wall and
DNA chains particles if any will be set, and then all fluid particles are initially
located at the sites of a face-centered cubic (FCC) lattice
In the main program, the initial velocities of fluid particles are set randomly
according to the given temperature The velocities of wall particles are set at zero At
the beginning of simulation the fluid particles are allowed to move without applying
any external forces until a thermodynamic equilibrium state is reached Then the
external force field is applied to fluid particles and the non-equilibrium simulation
starts
In this kind of simulation, computing the interaction forces between particles takes
the most computational time To cope with this problem, here a cell sub-division and
linked-list method described by Rapaport [28] is applied In this method, firstly the
Trang 34particles with the cells in which they reside at any given instance The linked list
therefore associates a pointer with each data item and to provide a non-sequential
path through the data Thus it needs only a one dimension array to store the list and
makes the search of neighboring particles more efficiently
Three parts will be discussed below: firstly the boundary conditions used in this thesis
are outlined, afterwards the effects of two DPD parameters on the simulation are
analyzed, then the simulation results of simple DPD particles in concentric/eccentric
flows are presented The simulation results of DNA polymer chains suspension in
concentric/eccentric flows will be presented in the next chapter
3.1 Implementation of non-slip boundary condition in DPD
As with any other methods in computational fluid dynamics, the issue of boundary
conditions has to be addressed in DPD Until now, the boundary conditions in DPD
are usually treated in two ways:
1 In order to simulate a shear flow such as that generated in a Couette geometry,
the Lees-Edward technique has been used [3, 6, 19], which is a way of avoiding
the modelization of physical boundaries
2 When considering the boundary conditions on the surface of solid objects as in
the modelization of colloidal suspensions, the method of “freezing” some
portions of the fluid described by DPD particles has been used [7, 29, 30, 31] In
Trang 35this model, those particles are fixed but still can interact with other free particles
[32]
Due to the soft repulsion between DPD particles, it is difficult to prevent fluid
particles from penetrating the wall particles Near-wall particles may not be slowed
down enough and slip may then occur To avoid this, higher density of wall particles
and larger repulsive forces have to be adopted to strengthen the wall effects This,
however, results in large density distortions in the flow field, which is similar to what
happened in MD simulation Special treatments have been proposed to implement no
slip boundary condition in DPD simulation without using frozen wall particles
Revenga et al [33, 34] used effective forces to represent the effect of wall on fluid
particles instead of using wall particles For planar wall, the effective forces can be
obtained analytically But these forces are not sufficient to prevent fluid particles from
crossing the wall When particles cross the wall, a wall reflection is used to reflect
particles back to the fluid However, a slip velocity appears at the wall if the wall
density is equal to that of the fluid, and no slip results only if the wall has a much
higher density than that of the fluid To cope with this problem, Willemsen et al [35]
added an extra layer of particles outside of the simulation domain The position and
velocity of particles in this layer are determined by the particles inside the simulation
domain near the wall, such that the mean velocity of a pair of particles inside and
outside the wall satisfies the given boundary conditions Furthermore, to reduce the
Trang 36the particles being located between r c and 2r c from the boundary into this layer, and
considering the repulsive forces between those particles and free particles Obviously,
this method is quite expensive computationally and very difficult to use for the
complex surface of solid objects such as a sphere or cylinder
Since the effective forces are not sufficient for keeping the fluid confined and one has
to specify what happens when a DPD particle crosses the line that defines the position
of the wall Normally, there are three different possibilities:
1 Specular reflection: such that the parallel component of the momentum of the
particles is conserved and the normal components is reversed
2 Maxwellian reflection: where the particles are introduced back into the system
according to a Maxwellian distribution of velocities centered at the velocity of
the wall
3 Bounce back reflection: in which both components of the velocity are reversed
In [34], Revenga et al compared these three methods, and they found that for small
is the thermal velocity), slip appears in specular and Maxwellian reflections and the
the bounce back scheme produces an anomalous temperature behavior
Trang 37Later, considering the merits and disadvantages of above methods, Fan et al [15]
present their model based on the above discussions and obtained good simulation
results for Posieuille flow They still used frozen particles to represent the wall, but
near the wall a thin layer is assumed where the no slip boundary condition holds To
meet this boundary condition, they enforced a random velocity distribution in this
layer with zero mean and corresponding to the given temperature Similar to Revenga
et al.’s reflection law, Fan et al [15] further required that particles within this layer
always leave the wall The velocity of particle i in the layer is
into the fluid domain The above equation means that the normal velocity component
of fluid particles within the assumed thin layer will always move away from the wall
and the parallel component of the momentum of the particle is conserved
In this section, a new boundary condition model of the frozen particles to represent
the wall is presented which satisfies no-slip boundary condition and also has its own
merits Firstly, this boundary condition model is outlined, and then simulation results
from this boundary condition are compared with those of Fan et al.’s model [15] in
two cases: Poisseuille flow and circular Couette flow
3.1.1 Boundary condition used in this thesis
Trang 38interior; In order to produce a non slip effect, each particle colliding with the wall has
all memory of its previous velocity erased, and is reflected back into the system with a
new velocity having a random direction and fixed magnitude which is set to a value
corresponding to the wall temperature In addition, for the wall of the rotating
cylinder the local (tangential) wall velocity is added to yield a new velocity vector
This mechanism is sufficient to drive the fluid rotation and dissipate the thermal
energy generated by the sheared flow
The main differences from Fan et al’s model [15] lie in:
1 Only particles which intend to cross the wall boundary instead of all particles
lying within the thin layer are imposed with a new velocity corresponding to
the given temperature;
2 In addition, the updated positions of those reflected particles are traced
accurately in the program rather than being given an approximate position as
noted by Rapaport [28] This idea can be shown clearly with Figure 4:
Different with Maxwellian reflection scheme (noted above), in which the new
velocity is distributed with the random directions, the boundary condition used here
retains the parallel part of the old velocity and makes the vertical vector point into the
interior area (see Equation (22))
Trang 39(a) t0→ + ∆t0 λ t (0< < with the λ 1)
original velocity
the new velocity
Figure 4 Illustration of the boundary reflection
3.1.2 Comparison of boundary conditions: Poisseuille flow
Fan et al.’s boundary model [15] gives a rather good simulation results for simple
Poisseuille flows, but in their article an obvious fluctuation of density and pressure in
the region near the wall was noted, although this fluctuation is not as severe as what
was predicted by Molecular Dynamics simulation In this section, to make a
convincing comparison, the same parameters are selected as noted in [15] The
wall particles are located in three layers parallel to the (x, y) plane in each side The
boundary condition is applied to fluid boundaries in the X and Y directions The
gravity force g=0.02 is applied to drive the flow The simulation region is divided into
300 bins in the z- direction, of which 278 bins are located in the fluid domain, and
others are in the wall domain All local flow properties are obtained by averaging the
Trang 40In Figure 5, 6, 7 and 8, the fully developed velocity, temperature, shear stress and
normal stress (N1 and N2) profiles are depicted Similar to what have been presented
in [15], these profiles simulated with the new boundary condition coincide excellently
with the analytical results We could find that the velocity and shear stress profiles
agree with the Navier-Stokes analytical solution accurately except for the region near
the wall surfaces; the temperature profile is uniform across the channel; the first (N1)
and second (N2) normal stress difference profiles are almost zero along the z-
direction which confirms that the simple DPD particle solvent is a Newtonian fluid,
which is also a main conclusion of Fan et al.’s paper [15]
While in Figure 9, we could find the density fluctuation near the wall region is
reduced significantly (about 40%) with the new boundary condition As a result, the
distortion of the pressure is also alleviated greatly as shown in Figure 10 So with the
new implementation for modeling the boundary, a better simulation result is obtained
without increasing the computation effort If the wall particle density is retained, a
better result may be reached if we find out more precise parameter such as the